Lateral neck X-ray provides a diagnostic clue in a child presenting with dyspnoea and stridor

AbstractLiver cirrhosis in infancy can be secondary to various etiologies such as biliary atresia, familial cholestatic and metabolic disorders. Wolman's disease (WD) is a lysosomal storage disorder caused by the absence of lysosomal acid lipase enzyme activity and a significant association with infantile cholestasis and cirrhosis. We encountered an infant presenting with advanced cirrhosis and decompensation having splenomegaly for which the underlying etiology was found to be WD and the diagnostic clue came from abdominal X-ray showing bilateral adrenal calcifications. The diagnosis was confirmed by genetic analysis. The outcome was poor and died before 6 months of age without enzyme replacement therapy or hematopoietic stem cell transplantation.

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Diagnostic value of the upper lip bite test in predicting difficulty in intubation with head and neck landmarks obtained from lateral neck X-ray

Indian Journal of Anaesthesia ◽

10.4103/0019-5049.118567 ◽

2013 ◽

Vol 57 (4) ◽

pp. 381 ◽

Cited By ~ 6

Author(s):

ZahidHussain Khan ◽

Shahriar Arbabi

Keyword(s):

Head And Neck ◽

Diagnostic Value ◽

Lateral Neck ◽

Upper Lip ◽

X Ray

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Space and Time Distribution of Hard X-Ray Emission in a Loop at the Beginning of a Flare

International Astronomical Union Colloquium ◽

10.1017/s0252921100025446 ◽

1994 ◽

Vol 144 ◽

pp. 275-277

Author(s):

M. Karlický ◽

J. C. Hénoux

Keyword(s):

Time Distribution ◽

Electron Bombardment ◽

Spatial Evolution ◽

Superthermal Electrons ◽

Flare Loop ◽

X Ray ◽

Superthermal Electron ◽

Flare Loops ◽

Chromospheric Evaporation ◽

Temporal And Spatial

AbstractUsing a new ID hybrid model of the electron bombardment in flare loops, we study not only the evolution of densities, plasma velocities and temperatures in the loop, but also the temporal and spatial evolution of hard X-ray emission. In the present paper a continuous bombardment by electrons isotropically accelerated at the top of flare loop with a power-law injection distribution function is considered. The computations include the effects of the return-current that reduces significantly the depth of the chromospheric layer which is evaporated. The present modelling is made with superthermal electron parameters corresponding to the classical resistivity regime for an input energy flux of superthermal electrons of 109erg cm−2s−1. It was found that due to the electron bombardment the two chromospheric evaporation waves are generated at both feet of the loop and they propagate up to the top, where they collide and cause temporary density and hard X-ray enhancements.

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Some Problems in Understanding the Solar Corona

International Astronomical Union Colloquium ◽

10.1017/s025292110002491x ◽

1994 ◽

Vol 144 ◽

pp. 1-9

Author(s):

A. H. Gabriel

Keyword(s):

Solar Corona ◽

Solar Atmosphere ◽

Theoretical Modelling ◽

Total System ◽

Major Advance ◽

X Ray ◽

Proper Perspective ◽

Space Observations

The development of the physics of the solar atmosphere during the last 50 years has been greatly influenced by the increasing capability of observations made from space. Access to images and spectra of the hotter plasma in the UV, XUV and X-ray regions provided a major advance over the few coronal forbidden lines seen in the visible and enabled the cooler chromospheric and photospheric plasma to be seen in its proper perspective, as part of a total system. In this way space observations have stimulated new and important advances, not only in space but also in ground-based observations and theoretical modelling, so that today we find a well-balanced harmony between the three techniques.

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